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Geomagnetically induced currents (GIC) registered at the VKH station are analyzed during the intervals of Pc5/Pi3 activity at IMAGE network during the year 2015, near the maximum of 24-th Solar cycle. It is shown that geomagnetic pulsations, developing at recovery phase of geomagnetic storms and at non-storm intervals lead to long-lasting intervals of potentially dangerous GICs. Interdependence of GIC and pulsation parameters are analyzed under different space weather conditions, including the influence of pulsations’ spectra, polarization, and spatial distribution.